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	射电望远镜天线主反射面面形测量方法综述期刊论文 OAI收割中国科学: 物理学力学天文学, 2024, 卷号: 54, 期号: 1, 页码: 219503 作者: 班友; 刘源杰; 王娜; 古丽加依娜・哈再孜汗; 冯树飞 \| 收藏 \| 浏览/下载：1/0 \| 提交时间：2025/06/05 射电望远镜面形精度面形测量方法 Radio telescope reflector accuracy reflector measurement method
	Analysis of Coaxiality Error Induced by the Cube Corner Retro-Reflector Geometrical and Assembly Errors of an Acquisition, Pointing, and Tracking System 期刊论文 OAI收割 PHOTONICS, 2023, 卷号: 10, 期号: 10 作者: Li, Daquan; Mao, Zhaoyong; Sun, Lijuan; Zhang, Haifeng; Zhang, Furui \| 收藏 \| 浏览/下载：29/0 \| 提交时间：2023/11/17 space laser communication coaxiality cube corner retro-reflector assembly error beam-pointing accuracy
	Hybrid-panel-based new design idea for large reflector antenna 期刊论文 OAI收割 SCIENCE CHINA-TECHNOLOGICAL SCIENCES, 2022, 页码: 12 作者: Lian PeiYuan; Yan YueFei; Wang CongSi; Qin Long; Xue Song \| 收藏 \| 浏览/下载：47/0 \| 提交时间：2023/02/28 reflector antenna hybrid panel actuator distribution adjustment strategy surface accuracy power pattern
	Relaxing the Small Facet Size Requirement for the Far-Field Calculation of Large Reflector Antennas 期刊论文 OAI收割 Ieee Transactions on Antennas and Propagation, 2021, 卷号: 69, 期号: 8, 页码: 4261-4268 作者: Ban, You; Feng, Shufei; Lou, Shunxi; Xiang, Binbin; Duan, Baoyan \| 收藏 \| 浏览/下载：29/0 \| 提交时间：2022/06/30 Reflector antennas Systematics Aperture antennas Optimization Surface waves Surface fitting Mechanical engineering Accuracy far-field pattern large reflector antenna design Engineering Telecommunications
	Effect of Facet Displacement on Radiation Field and Its Application for Panel Adjustment of Large Reflector Antenna 期刊论文 OAI收割 Chinese Journal of Mechanical Engineering, 2017, 卷号: 30, 期号: 3, 页码: 578-586 作者: Wang, Wei; Lian, Peiyuan; Zhang, Shuxin; Xiang, Binbin; Xu, Qian \| 收藏 \| 浏览/下载：50/0 \| 提交时间：2019/12/09 Reflector antennas Surface accuracy Radiation field Reflector antenna mechanical factors Electromechanical effects Panel adjustment Singular value decomposition (SVD) microwave holography surface measurement radio telescope deformation metrology matrix Engineering
	Experiments on the dish verification antenna china for the SKA 期刊论文 OAI收割 EXPERIMENTAL ASTRONOMY, 2016, 卷号: 42, 期号: 3, 页码: 301-317 作者: Chai, Xiaoming; Liu, Bin; Yu, Lei; Yu, Shenghua; Wu, Di \| 收藏 \| 浏览/下载：23/0 \| 提交时间：2019/04/08 Single-piece CFRP reflector Pointing accuracy Aperture efficiency DVA-C SKA
	Experiments on the dish verification antenna china for the SKA 期刊论文 OAI收割 EXPERIMENTAL ASTRONOMY, 2016, 卷号: 42, 期号: 3, 页码: 301-317 作者: Chai, Xiaoming; Liu, Bin; Yu, Lei; Yu, Shenghua; Wu, Di 收藏 \| 浏览/下载：33/0 \| 提交时间：2017/03/01 Single-piece CFRP reflector Pointing accuracy Aperture efficiency DVA-C SKA
	Design and experimental research of a new type focus mechanism used in space-based telescope (EI CONFERENCE) 会议论文 OAI收割 2012 9th IEEE International Conference on Mechatronics and Automation, ICMA 2012, August 5, 2012 - August 8, 2012, Chengdu, China 作者: Wang D. 收藏 \| 浏览/下载：40/0 \| 提交时间：2013/03/25 The position of focal plane will be changed because of temperature fluctuation and vacuum environment. In order to make the telescope work well positioning accuracy of the mechanism is 0.008mm. The performance satisfies the need of precision a focusing mechanism is needed. To majority of large space-based telescopes and the scheme design is reasonable and practicable. 2012 IEEE. the general way to do this would be to use a reflector which was located in the backfocal distance. One of typical schemes of this mechanism was introduced however because of the big axial size the mechanism can't be used when the size of the enclosure was limited. A new type of focusing mechanism was introduced which has such advantages of small size high accuracy and low mass. The design and test methods had been discussed. According to the results the repeatability positioning accuracy is 0.0025mm
	Research on the support structure of the primary mirror of large-aperture telescope (EI CONFERENCE) 会议论文 OAI收割 3rd International Symposium on Advanced Optical Manufacturing and Testing Technologies, AOMATT 2007: Large Mirrors and Telescopes, July 8, 2007 - July 12, 2007, Chengdu, China Yang W.; Jingxu Z. 收藏 \| 浏览/下载：32/0 \| 提交时间：2013/03/25 Large-aperture telescope can be used in surveying battlefield researching landform searching object real-time monitoring imaging detecting and identifying spatial targets and so on. A large-aperture telescope for achieving high resolution power is designed to monitor spatial target and image in real time. Real-time monitoring plays an important role in military conflicts. The orbit parameter of object quantity geometrical shape parameter and so on can be obtained by detect spatial target. With the development of optical technology people require larger aperture in optics-electronic (OE) system. By increasing optical aperture the ability of collecting light and resolution power in the system can be enhanced. But the support structure of the primary mirror of large-aperture telescope will be a very difficult problem. With the increase of primary mirror aperture the weight of the primary mirror will become larger than before. The root mean square (rms) of the primary mirror is affected by many factors such as deadweight deformation of heat environment and so on. Due to the primary mirror of telescope is an important component of telescope system. By reducing the weight of primary mirror precision of the system is ensured. During the designing phase one can consider the supporting project of the primary mirror synthetically and analyze it roundly according to technical requirement of optical system and the effect factors. The final structural design can be reasonable. In an astronomical telescope the surface of reflector is an important part for collecting dark radiation of celestial bodies. Its surface shape will have an effect on collecting efficiency of telescope radiant energy directly. So the rms must be very high. Optical system of large aperture small wavelength and small focus can receive maximal light intensity. For ground-based optical astronomical telescope the design proposed in the paper can satisfy the requirement of the possible minimum atmosphere seeing at astronomical observatory site and exert the use efficiency of the telescope adequately. So the accuracy of the traditional surface of reflector can assure that 90% of all the light energy can be focused on within the angle diameter range of the minimum atmosphere seeing then 100% of light energy should be focused on the angle diameter range of minimum atmosphere seeing. Because the rms of mirror is very high precise surface machining and accurate the support of mirror are very important tasks during designing and manufacturing the telescope. In the paper various support techniques of a large-aperture telescope primary mirror are discussed and a 3.5 meter telescope system at the Starfire Optical Range (SOR) overviewed simply which was operated by the Directed Energy Directorate of the Air Force Research Laboratory Kirtland AFB NM USA from the ground-based O-E system for the observations of spatial target. We also analyze Theoretical elastic deformation of the Steward Observatory 2.3 meter mirror is analyzed.